Sub-Alfvénic Turbulence: Magnetic-to-kinetic Energy Ratio, Modification of Weak Cascade, and Implications for Magnetic Field Strength Measurements

We study the properties of sub-Alfvénic magnetohydrodynamic (MHD) turbulence, i.e., turbulence with Alfvén mach number M _A = V _L / V _A < 1, where V _L is the velocity at the injection scale and V _A is the Alfvén velocity. We demonstrate that MHD turbulence can have different properties, depen...

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Podrobná bibliografie
Hlavní autoři: A. Lazarian, Ka Wai Ho, Ka Ho Yuen, Ethan Vishniac
Médium: Článek
Jazyk:English
Vydáno: IOP Publishing 2024-01-01
Edice:The Astrophysical Journal
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On-line přístup:https://doi.org/10.3847/1538-4357/ad8d49